{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:EXI2X3FOHFVIN2A7XLVT6L4O63","short_pith_number":"pith:EXI2X3FO","schema_version":"1.0","canonical_sha256":"25d1abecae396a86e81fbaeb3f2f8ef6cc2d3d56d1f8b207ffbac0aa52eac1e1","source":{"kind":"arxiv","id":"2105.02663","version":2},"attestation_state":"computed","paper":{"title":"SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Sp\\'erone-Longin, D. Zaritsky, F. Combes, G. Castignani, G. De Lucia, G. Rudnick, M. Krips, P. Jablonka, R. A. Finn, T. Desjardins, V. Desai","submitted_at":"2021-05-06T13:44:45Z","abstract_excerpt":"This paper is the second of a series that tackles the properties of molecular gas in galaxies residing in clusters and their related large-scale structures. Out of 21 targeted fields, 19 galaxies were detected in CO(3-2) with the Atacama Large Millimeter Array (ALMA), including two detections within a single field. These galaxies are either bona fide members of the CL1301.7$-$1139 cluster ($z=0.4828$, $\\sigma_{cl}=681$ km s$^{-1}$), or located within $\\sim 7 \\times R_{200}$, its virial radius. They have been selected to sample the range of photometric local densities around CL1301.7$-$1139, wi"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2105.02663","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2021-05-06T13:44:45Z","cross_cats_sorted":[],"title_canon_sha256":"eb678eb3702772f8e10f68f8aa707b42cf5b8cf24753065c0a272ace60aebec7","abstract_canon_sha256":"f239756d726098f5d66139c7d5784c9155d9c443c1a02d7d003a33abb6a18ec9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:21:48.227104Z","signature_b64":"TkSjRW4YaE5qkwKL3n/DY8IcAKKqyBIC0HzZHg/boAihXqcBUqKsocDg89/gWcxEKolpldtlxcXtnVpDV5KKDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"25d1abecae396a86e81fbaeb3f2f8ef6cc2d3d56d1f8b207ffbac0aa52eac1e1","last_reissued_at":"2026-07-05T03:21:48.226694Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:21:48.226694Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"SEEDisCS II. Molecular gas in galaxy clusters and their large scale structure: low gas fraction galaxies, the case of CL1301.7$-$1139","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Sp\\'erone-Longin, D. Zaritsky, F. Combes, G. Castignani, G. De Lucia, G. Rudnick, M. Krips, P. Jablonka, R. A. Finn, T. Desjardins, V. Desai","submitted_at":"2021-05-06T13:44:45Z","abstract_excerpt":"This paper is the second of a series that tackles the properties of molecular gas in galaxies residing in clusters and their related large-scale structures. Out of 21 targeted fields, 19 galaxies were detected in CO(3-2) with the Atacama Large Millimeter Array (ALMA), including two detections within a single field. These galaxies are either bona fide members of the CL1301.7$-$1139 cluster ($z=0.4828$, $\\sigma_{cl}=681$ km s$^{-1}$), or located within $\\sim 7 \\times R_{200}$, its virial radius. They have been selected to sample the range of photometric local densities around CL1301.7$-$1139, wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.02663","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2105.02663/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2105.02663","created_at":"2026-07-05T03:21:48.226750+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.02663v2","created_at":"2026-07-05T03:21:48.226750+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.02663","created_at":"2026-07-05T03:21:48.226750+00:00"},{"alias_kind":"pith_short_12","alias_value":"EXI2X3FOHFVI","created_at":"2026-07-05T03:21:48.226750+00:00"},{"alias_kind":"pith_short_16","alias_value":"EXI2X3FOHFVIN2A7","created_at":"2026-07-05T03:21:48.226750+00:00"},{"alias_kind":"pith_short_8","alias_value":"EXI2X3FO","created_at":"2026-07-05T03:21:48.226750+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63","json":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63.json","graph_json":"https://pith.science/api/pith-number/EXI2X3FOHFVIN2A7XLVT6L4O63/graph.json","events_json":"https://pith.science/api/pith-number/EXI2X3FOHFVIN2A7XLVT6L4O63/events.json","paper":"https://pith.science/paper/EXI2X3FO"},"agent_actions":{"view_html":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63","download_json":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63.json","view_paper":"https://pith.science/paper/EXI2X3FO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.02663&json=true","fetch_graph":"https://pith.science/api/pith-number/EXI2X3FOHFVIN2A7XLVT6L4O63/graph.json","fetch_events":"https://pith.science/api/pith-number/EXI2X3FOHFVIN2A7XLVT6L4O63/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63/action/storage_attestation","attest_author":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63/action/author_attestation","sign_citation":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63/action/citation_signature","submit_replication":"https://pith.science/pith/EXI2X3FOHFVIN2A7XLVT6L4O63/action/replication_record"}},"created_at":"2026-07-05T03:21:48.226750+00:00","updated_at":"2026-07-05T03:21:48.226750+00:00"}